Zorotovic M.; Schreiber M.R.; Gansicke B.T.; Rebassa-Mansergas A.; Nebot Gomez-Moran A.; Southworth J.; Schwope A.D.; Pyrzas S.; Rodriguez-Gil P.; Schmidtobreick L.; Schwarz R.; Tappert C.; Toloza O.; Vogt N.
(2014-04-04)
Context. Post-common-envelope binaries (PCEBs) consisting of a white dwarf (WD) and a main-sequence secondary star are ideal systems to constrain models of common-envelope (CE) evolution. Until very recently, observed ...